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The early-contact system BH Centauri:UBV photometry
Authors:R F Sistero  A Grieco  B Candellero
Institution:1. Department of Physics, University of Gorakhpur, Gorakhpur, India
Abstract:Some basic equations pertaining to the accretion of perfect magnetofluid on compact objects are derived without assuming that the flow is purely circular or purely radial. In addition, we assume that the magnetofluid exerts negligible self-gravitation and that its flow is stationary and axisymmetric. We restrict ourselves to the case of ‘stiff’ or ‘incompressible’ fluid with an equation of state: pressure = energy-density.
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